{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:4MUYFNOZWOWSF2ZB5H5AG3DJIJ","short_pith_number":"pith:4MUYFNOZ","schema_version":"1.0","canonical_sha256":"e32982b5d9b3ad22eb21e9fa036c69424ffed01d5f89f42e593dfa12a98cd5af","source":{"kind":"arxiv","id":"2109.10920","version":3},"attestation_state":"computed","paper":{"title":"The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis \\`a vis One-Dimensional, Massive-star Supernova Progenitor Models","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Adam Burrows, David Vartanyan, Matthew S.B. Coleman","submitted_at":"2021-09-22T18:00:04Z","abstract_excerpt":"The explosion outcome and diagnostics of core-collapse supernovae depend sensitively on the nature of the stellar progenitor, but most studies to date have focused exclusively on one-dimensional, spherically-symmetric massive star progenitors. We present some of the first core-collapse supernovae simulations of three-dimensional massive star supernovae progenitors, a 12.5- and a 15-M$_{\\odot}$ model, evolved in three-dimensions from collapse to bounce through explosion with the radiation-hydrodynamic code F{\\sc{ornax}}. We compare the results using those starting from three-dimensional progeni"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2109.10920","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2021-09-22T18:00:04Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"e45ad38249a582e3659a1b03b05a3eead052e14c932927655e0fd06da06f985b","abstract_canon_sha256":"265b59bda7fb3d438c7744ca332a759c9668fafe67debbc8195360310a4c4390"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:48:08.239128Z","signature_b64":"ks8g9FoLuvHvsiJUDOhm+ZGYHHauAzXR5vqrM5VrZNnukugqN///eYhdI0XRpYQDtRuwY7Of7+QgzLf/tI6aBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e32982b5d9b3ad22eb21e9fa036c69424ffed01d5f89f42e593dfa12a98cd5af","last_reissued_at":"2026-07-05T03:48:08.238692Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:48:08.238692Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis \\`a vis One-Dimensional, Massive-star Supernova Progenitor Models","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Adam Burrows, David Vartanyan, Matthew S.B. Coleman","submitted_at":"2021-09-22T18:00:04Z","abstract_excerpt":"The explosion outcome and diagnostics of core-collapse supernovae depend sensitively on the nature of the stellar progenitor, but most studies to date have focused exclusively on one-dimensional, spherically-symmetric massive star progenitors. We present some of the first core-collapse supernovae simulations of three-dimensional massive star supernovae progenitors, a 12.5- and a 15-M$_{\\odot}$ model, evolved in three-dimensions from collapse to bounce through explosion with the radiation-hydrodynamic code F{\\sc{ornax}}. We compare the results using those starting from three-dimensional progeni"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2109.10920","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2109.10920/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2109.10920","created_at":"2026-07-05T03:48:08.238745+00:00"},{"alias_kind":"arxiv_version","alias_value":"2109.10920v3","created_at":"2026-07-05T03:48:08.238745+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2109.10920","created_at":"2026-07-05T03:48:08.238745+00:00"},{"alias_kind":"pith_short_12","alias_value":"4MUYFNOZWOWS","created_at":"2026-07-05T03:48:08.238745+00:00"},{"alias_kind":"pith_short_16","alias_value":"4MUYFNOZWOWSF2ZB","created_at":"2026-07-05T03:48:08.238745+00:00"},{"alias_kind":"pith_short_8","alias_value":"4MUYFNOZ","created_at":"2026-07-05T03:48:08.238745+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06664","citing_title":"Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors","ref_index":293,"is_internal_anchor":true},{"citing_arxiv_id":"2606.06580","citing_title":"Neutrino mass ordering from the next Galactic supernova at DUNE, HK, and JUNO","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04896","citing_title":"Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors","ref_index":37,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ","json":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ.json","graph_json":"https://pith.science/api/pith-number/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/graph.json","events_json":"https://pith.science/api/pith-number/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/events.json","paper":"https://pith.science/paper/4MUYFNOZ"},"agent_actions":{"view_html":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ","download_json":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ.json","view_paper":"https://pith.science/paper/4MUYFNOZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2109.10920&json=true","fetch_graph":"https://pith.science/api/pith-number/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/graph.json","fetch_events":"https://pith.science/api/pith-number/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/action/storage_attestation","attest_author":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/action/author_attestation","sign_citation":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/action/citation_signature","submit_replication":"https://pith.science/pith/4MUYFNOZWOWSF2ZB5H5AG3DJIJ/action/replication_record"}},"created_at":"2026-07-05T03:48:08.238745+00:00","updated_at":"2026-07-05T03:48:08.238745+00:00"}